Efficiency of charged-particle acceleration by shocks in supernova remnants and in solar flares
Journal Article
·
· Sov. Astron. Lett. (Engl. Transl.); (United States)
OSTI ID:6249417
Cosmic-ray acceleration by shocks in supernova envelopes can explain certain properties of the radio emission of old SNRs. The pressure of the accelerated particles should contribute little to the envelope dynamics. An estimate is obtained for the level of turbulence required for this acceleration mechanism to operate in solar flares.
- Research Organization:
- Institute of General Physics, USSR Academy of Sciences, Moscow
- OSTI ID:
- 6249417
- Journal Information:
- Sov. Astron. Lett. (Engl. Transl.); (United States), Vol. 10:4
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COSMIC RADIATION
ACCELERATION
SOLAR FLARES
SHOCK WAVES
SOLAR PARTICLES
SUPERNOVA REMNANTS
COSMIC RAY PROPAGATION
DYNAMICS
EFFICIENCY
PLASMA ACCELERATION
RADIATION PRESSURE
RADIOWAVE RADIATION
SOLAR RADIATION
TURBULENCE
COSMIC RADIO SOURCES
ELECTROMAGNETIC RADIATION
IONIZING RADIATIONS
MECHANICS
RADIATIONS
SOLAR ACTIVITY
STELLAR RADIATION
640104* - Astrophysics & Cosmology- Solar Phenomena
640101 - Astrophysics & Cosmology- Cosmic Radiation
GENERAL PHYSICS
COSMIC RADIATION
ACCELERATION
SOLAR FLARES
SHOCK WAVES
SOLAR PARTICLES
SUPERNOVA REMNANTS
COSMIC RAY PROPAGATION
DYNAMICS
EFFICIENCY
PLASMA ACCELERATION
RADIATION PRESSURE
RADIOWAVE RADIATION
SOLAR RADIATION
TURBULENCE
COSMIC RADIO SOURCES
ELECTROMAGNETIC RADIATION
IONIZING RADIATIONS
MECHANICS
RADIATIONS
SOLAR ACTIVITY
STELLAR RADIATION
640104* - Astrophysics & Cosmology- Solar Phenomena
640101 - Astrophysics & Cosmology- Cosmic Radiation